This release includes the PACS photometric and spectroscopic data from OT2_jwardlow_1 that are published in Wardlow et al., 2017, ApJ, 837, 12. Please reference Wardlow et al., 2017, ApJ, 837, 12 when using the data and see that paper for further details of the target selection and data reduction. The release includes: - This README file - The published paper: wardlow17_published.pdf - PACS photometric maps (70 and 160 micron) from Program ID OT2_jwardlow_1: [target]_[waveband].fits.gz - PACS spectroscopic cubes from Program ID OT2_jwardlow_1: [target]_main_[targetedline]_cube.fits.gz for targeted emission lines, and [target]_2ndorder_[targetedline]_cube.fits.gz (where the second order cubes are available) As the wavelength coverage of the second order data is offset from the primarily targeted transitions, no line emission is typically expected in those data cubes (NB: [OIV]+[FeII]26micron that is observed in the second order of [OIII]52micron observations are labelled as "main_OIV26") All data files are all gzipped for easy download. Targets are listed in Wardlow et al. 2017, table 1. Briefly (formal name, short names, line transitions observed): H-ATLAS J142935.3−002836 , G15v2.19 G15.DR1.14 , [OI]63micron [NIII]57micron H2S(0) H-ATLAS J085358.9+015537 , G09v1.40 G09.DR1.35 , [OI]63micron [SiII]34micron [OIII]52micron [NIII]57micron [OIV]+[FeII]26micron H2S(0) H-ATLAS J115820.2−013753 , G12v2.257 G12.DR1.379 , [SIII]33micron [SiII]34micron [OIII]52micron [OIV]+[FeII]26micron H-ATLAS J133649.9+291801 , NGP.NA.144 , [OI]63micron [SIII]33micron [SiII]34micron [OIII]52micron [NIII]57micron [OIV]+[FeII]26micron H2S(1) H-ATLAS J134429.4+303036 , NGP.NA.56 , [OI]63micron [SIII]33micron [SiII]34micron [OIII]52micron [NIII]57micron [OIV]+[FeII]26micron H2S(0) H2S(1) 1HerMES S250 J022016.5−060143, HXMM01 , [OI]63micron [SIII]33micron [SiII]34micron [OIII]52micron [OIV]+[FeII]26micron H2S(1) H-ATLAS J084933.4+021443 , G09v1.124 G09.DR1.131 , [SIII]33micron [SiII]34micron [OIII]52micron [OIV]+[FeII]26micron H2S(1) H-ATLAS J141351.9−000026 , G15v2.235 G15.DR1.265 , [SIII]33micron [SiII]34micron [OIII]52micron [OIV]+[FeII]26micron H2S(1) H-ATLAS J091840.8+023047 , G09v1.326 G09.DR1.437 , [SIII]33micron [OIII]52micron [OIV]+[FeII]26micron H-ATLAS J133008.4+245900 , NGP.NB.78 , [SIII]33micron [SiII]34micron H2S(0) H-ATLAS J113526.3−014605 , G12v2.43 G12.DR1.80 , [SIII]33micron [SiII]34micron [OIV]+[FeII]26micron H2S(0) H-ATLAS J114637.9−001132 , G12v2.30 G12.DR1.33 , [SIII]33micron [SiII]34micron [OIV]+[FeII]26micron H2S(0) H2S(1) 1HerMES S250 J143330.8+345439, HBoötes01 , [SIII]33micron [SiII]34micron H2S(0) Targets are candidate gravitationally lensed galaxies identified in the Herschel HerMES and H-ATLAS surveys (Oliver et al. 2012; Eales et al. 2010; Negrello et al. 2010; Wardlow et al. 2013; Nayyeri et al. 2016; Negrello et al. 2017), with robust spectroscopic redshifts, 250 micron fluxes >=100mJy, predicted 70 micron fluxes >=5mJy. The different transitions are selected for observation depending on source redshift (i.e. whether the redshifted line is accessible to PACS) and the likely required sensitivity (for details see Wardlow et al. 2017, Section 2.1). Photometric data (Details in Wardlow et al. 2017, Section 2.3): Simultaneous mini-scan maps at 70 and 160 micron are provided for each target. Observations were taken at the nominal scan speed of 20 arcsec per second with 3 arcmin scan legs, separated by 4 arcsec cross-scan steps. At least two orthogonal scans of each source were made. The data were processed from level 0 using the Herschel Interactive Processing Environment (Ott et al. 2010; HIPE) v12.1.0 with version 65.0 of the PACS calibration tree. Standard Herschel data-reduction procedures were used, via the standard IPIPE script for scan maps containing point or marginally extended sources. The cross-scans were combined during reduction, and we iteratively filtered using a signal-to-noise threshold to mask the sources during filtering. The final maps are each ~3.5arcmin x ~7.5arcmin with coverage >=90% of the maximum in the central ~0.5arcmin x ~1arcmin area. Each photometric fits file includes the data image, flag map, coverage map and history information in different extensions. Spectroscopic data (Details in Wardlow et al. 2017, Section 2.2): The spectroscopic observations were all taken in range scan mode with small chop/nod throws for background subtraction. The data were reduced using HIPE v12.1.0 with version 65.0 of the PACS calibration tree (although no significant differences are found comparing with the v14.0.1 pipeline processed data). Data processing is based on the HIPE V12.1.0 IPIPE Background Normalization data reduction script for "chop/nod range scan" data. This procedure is optimized for faint sources and uses the off-source positions to perform the background subtraction and calibrate the detector response. During flat fielding, we set the "upsample factor" to 1 (and use the default "oversample" of 2) to avoid introducing correlated noise, and mask the wavelength regions where spectral lines are expected. The final spectra are binned to be Nyquist sampled at the native PACS resolution. No point source correction or continuum subtraction is applied to the cubes provided here.